Thickness of Lunar Mare Basalts: New Results Based on Modeling the Degradation of Partially Buried Craters
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چکیده
منابع مشابه
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CLEMENTINE 2.7 μm DATA AND 70-CM EARTH-BASED RADAR DATA PROVIDE ADDITIONAL CONSTRAINTS FOR UVVIS-BASED ESTIMATES OF TiO2 CONTENT FOR LUNAR MARE BASALTS. J. J. Gillis, P. G. Lucey, B. A. Campbell, and B. R. Hawke, Hawaii Institute of Geophysics and Planetology, University of Hawaii, 1680 East-West Road, POST 515, Honolulu, HI 96822 ([email protected]), 2Center for Earth and Planetary Studie...
متن کاملDistinguishing high-alumina mare basalts using Clementine UVVIS and Lunar Prospector GRS data: Mare Moscoviense and Mare Nectaris
[1] High-alumina (HA) mare basalts are a unique group of the lunar sample collection. Sample geochemistry indicates that these basalts are derived from sources composed of late-stage cumulates from the Lunar Magma Ocean (LMO). Their aluminous nature suggests their sources contained significant plagioclase, which has implications regarding the efficiency of plagioclase separation from earlier fo...
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ژورنال
عنوان ژورنال: Journal of Geophysical Research: Planets
سال: 2019
ISSN: 2169-9097,2169-9100
DOI: 10.1029/2018je005872